Solar eclipse of October 25, 2022

A partial solar eclipse occurred at the Moon’s descending node of orbit on Tuesday, October 25, 2022, with a magnitude of 0.8623. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

The eclipse was visible from Europe, Central Asia, West Asia, South Asia and from Northeast Africa. The maximal phase of the partial eclipse occurred on the West Siberian Plain in Russia near Nizhnevartovsk, where more than 82% of the Sun was eclipsed by the Moon. In India, the Sun was eclipsed during sunset ranging from 58% in the north and around 2% in the south. From Western Europe it appeared to be around 15-30% eclipsed. It was visible between 08:58 UTC, the greatest point of eclipse occurred at 11:00 UTC and it ended at 13:02 UTC.

The eclipse was featured in Dune: Part Two, directed by Denis Villenueve. The film was recorded in the Jordanian Desert.

Gallery

• Telescopic view from Milton Keynes, England, 10:02 UTC
• From Novate Milanese, Italy, 10:08 UTC
• From Lutkówka, Poland, 10:11 UTC
• From Berlin, Germany, 10:24 UTC
• From Žilina, Slovak Republic, 10:39 UTC
• From Moscow, Russia, 10:47 UTC
• From Poltava, Ukraine, 10:48 UTC
• Telescopic view from Istanbul, Turkey, 11:02 UTC
• Observed in Kiryat Ata, Israel
• From Dushanbe, Tajikistan, 12:07 UTC
• From Bhubaneswar, India, 12:11 UTC
• Animation from Belfort, France
• A transit of a bird during the eclipse from Kumbakonam, India
• Birds passing by while eclipse is happening. Ankara, Turkey, at 10:43 UTC

Eclipse timing

Places experiencing partial eclipse

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Related eclipses

Eclipses in 2022

• A partial solar eclipse on April 30.
• A total lunar eclipse on May 16.
• A partial solar eclipse on October 25.
• A total lunar eclipse on November 8.

Metonic

• Preceded by: Solar eclipse of January 6, 2019
• Followed by: Solar eclipse of August 12, 2026

Tzolkinex

• Preceded by: Solar eclipse of September 13, 2015
• Followed by: Solar eclipse of December 5, 2029

Half-Saros

• Preceded by: Lunar eclipse of October 18, 2013
• Followed by: Lunar eclipse of October 30, 2031

Tritos

• Preceded by: Solar eclipse of November 25, 2011
• Followed by: Solar eclipse of September 23, 2033

Solar Saros 124

• Preceded by: Solar eclipse of October 14, 2004
• Followed by: Solar eclipse of November 4, 2040

Inex

• Preceded by: Solar eclipse of November 13, 1993
• Followed by: Solar eclipse of October 4, 2051

Triad

• Preceded by: Solar eclipse of December 25, 1935
• Followed by: Solar eclipse of August 26, 2109

Solar eclipses of 2022–2025

Saros 124

This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of totality was produced by member 39 at 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’s descending node of orbit.

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.